Document Type
Article
Publication Date
2009
Abstract
We report on a search for continuous gravitational wave emission from three recycled radio pulsars, performed by using the data of the resonant detector AURIGA. Given the spin rate of the selected targets – the isolated pulsar PSR J1939+2134 and the binary pulsars PSR J0024-7204J and PSR J0218+4232 – the expected frequency of the emitted gravitational waves falls in the high sensitivity range of the detector.
Digital Commons Citation
Mion, A.; M. J. Benacquista; M. Kramer; P. P. C. Freire; and Possenti, A., "A Search For Periodic Gravitational Waves From Three Recycled Pulsars Using The Auriga Detector - An Implementation Of A Modified Version Of The Unified Approach Method" (2009). Faculty & Staff Scholarship. 450.
https://researchrepository.wvu.edu/faculty_publications/450
Source Citation
A. Mion, ., M. J. Benacquista, ., M. Kramer, ., P. P. C. Freire, ., & A. Possenti, .(2009). A Search For Periodic Gravitational Waves From Three Recycled Pulsars Using The Auriga Detector - An Implementation Of A Modified Version Of The Unified Approach Method. Astronomy And Astrophysics, 504(2), 673-679. http://doi.org/10.1051/0004-6361/200911946